HOME

BACK

 

NGC 6553

GLOBULAR CLUSTER IN SAGITTARIUS (THE ARCHER)

(Image centered at: ra 18 h:09 m / dec - 25º 54')

 

 

 CLICK THE IMAGE FOR A HIGH RESOLUTION VIEW

 

100% LUMINANCE RESOLUTION

 

October - 2024, Home Backyard in Martinez, Buenos Aires, Argentina

 


 

DATA

TYPE: GLOBULAR CLUSTER CLASS V

APPARENT DIAMETER: 9.2 arc minutes

APPARENT MAGNITUDE (V): 8.6

DISTANCE: 19600 light years

 

IMAGE INFORMATION

INSTRUMENT: 6" ORION OPTICS UK (Ultra Grade Optics) w/Sky Watcher Coma Corrector (0.9x) working at at f4.5

CAMERA: QHY 183 MONO

MOUNT: VIXEN GDPX, OAG with QHY 5II Mono

FILTERS: BAADER LRGB Set

SKY CONDITIONS: urban skies - Bortle 8

EXPOSURES: LRGB (45,45,45,45)

 

OBJECT DESCRIPTION AND IMAGE SESSION

NGC 6553 is a globular cluster in the constellation Sagittarius and one of the last targets I have imaged in 2024 from this crowded star area.  It is a Shapley–Sawyer Concentration Class is XI, meaning the star concentration is very loose even at the center. The globular has stars of magnitude 20 and dimmer. It is located just over a degree southeast of Messier 8, the Lagoon Nebula. Unlike common globular clusters, NGC 6553 is relatively metal-rich, and there is evidence of at least two periods of star formation. Due to a complex star-forming record, the stars in the cluster are differing in composition, most notably in concentrations of sodium and aluminum.

 

NGC 6553 was discovered by German - British astronomer William Herschel on May the 22nd 1784. He described as a "Faint, large, irregularly round, inclining to milkyness 3 or 4' diameter, like a brush to a north preceding star, but probably unconnected."

 


 

NGC 6553 - GLOBULAR CLUSTER

CROPPED LUMINANCE AT 100% RESOLUTION